nerc.ac.uk

Life cycle of the QBO modulated 11-year solar cycle signals in the northern hemispheric winter

Lu, Hua ORCID: https://orcid.org/0000-0001-9485-5082; Gray, Lesley J.; Baldwin, Mark P.; Jarvis, Martin J.. 2009 Life cycle of the QBO modulated 11-year solar cycle signals in the northern hemispheric winter. Quarterly Journal of the Royal Meteorological Society, 135 (641). 1030-1043. 10.1002/qj.419

Before downloading, please read NORA policies.
[thumbnail of LuGrayBaldwinJarvis_qj419_NORA.pdf]
Preview
Text
LuGrayBaldwinJarvis_qj419_NORA.pdf

Download (2MB) | Preview

Abstract/Summary

This paper provides some insights on the quasi-biennial oscillation (QBO) modulated 11-year solar cycle (11-yr SC) signals in Northern Hemisphere (NH) winter temperature and zonal wind. Daily ERA-40 Reanalysis and ECMWF Operational data for the period of 1958-2006 were used to examine the seasonal evolution of the QBO-solar cycle relationship at various pressure levels up to the stratopause. The results show that the solar signals in the NH winter extratropics are indeed QBO-phase dependent, moving poleward and downward as winter progresses with a faster descent rate under westerly QBO than under easterly QBO. In the stratosphere, the signals are highly significant in late January to early March and have a life span of similar to 30-50 days. Under westerly QBO, the stratospheric solar signals clearly lead and connect to those in the troposphere in late March and early April where they have a life span of similar to 10 days. As the structure changes considerably from the upper stratosphere to the lower troposphere, the exact month when the maximum solar signals occur depends largely on the altitude chosen. For the low-latitude stratosphere, our analysis supports a vertical double-peaked structure of positive signature of the 11-yr SC in temperature, and demonstrates that this structure is further modulated by the QBO. These solar signals have a longer life span (similar to 3-4 months) in comparison to those in the extratropics. The solar signals in the lower stratosphere are stronger in early winter but weaker in late winter, while the reverse holds in the upper stratosphere. Copyright (C) 2009 Royal Meteorological Society

Item Type: Publication - Article
Digital Object Identifier (DOI): 10.1002/qj.419
Programmes: BAS Programmes > Polar Science for Planet Earth (2009 - ) > Climate
ISSN: 0035-9009
Additional Keywords: solar influences, climate variability, stratospheric circulation
NORA Subject Terms: Meteorology and Climatology
Atmospheric Sciences
Date made live: 08 Nov 2010 11:15 +0 (UTC)
URI: https://nora.nerc.ac.uk/id/eprint/11141

Actions (login required)

View Item View Item

Document Downloads

Downloads for past 30 days

Downloads per month over past year

More statistics for this item...